The sample of stars in the night sky is biased by luminosity and longevity. I'd be curious to see a distribution of stellar masses that compensates for these two biases. On such a chart, extrapolating the trend in the high-mass range just before the error bars become too large would tell us whether 30-solar-mass stellar remnants are expected or unexpected by observation data.
The sample of stars in the night sky is biased by luminosity and longevity. I'd be curious to see a distribution of stellar masses that compensates for these two biases. On such a chart, extrapolating the trend in the high-mass range just before the error bars become too large would tell us whether 30-solar-mass stellar remnants are expected or unexpected by observation data.